A hard X-ray view on two distant TeV-blazars

Details A hard X-ray view on two distant TeV-blazars A hard X-ray view on two distant TeV-blazars

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..518r&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc

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Active And Peculiar Galaxies And Related Systems, Quasars, Active Or Peculiar Galaxies, Objects, And Systems, X-Ray, Mossbauer, And Other Gamma-Ray Spectroscopic Analysis Methods

Scientific paper

We present a data set derived from ~50 ksec continuous Suzaku observations and covered with quasi-simultaneous TeV-observations (HESS, MAGIC) of two of the more distant TeV-blazars detected to date: 1ES 1101-232 and 1ES 1553+113. Both sources are found in a non-variable state with combined XIS-PIN spectra indicating downward curvature up to several tens of keV. 1ES 101-232 was found in a quiet state with the lowest X-ray flux ever measured. We discuss the contemporaneous broadband spectral energy distribution (SED) of both sources and implications from absorption in the EBL for the redshift of 1ES 1553+113.

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